PPT-Computational needs at INFN

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S Farinon A Bersani B Caiffi A Gagno F Levi D Novelli A Pampaloni 11092023 ROXIE Users Workshop 11092023 ROXIE Users Workshop ROXIE Version 1021 2D amp 3D magnet

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Computational needs at INFN: Transcript

S Farinon A Bersani B Caiffi A Gagno F Levi D Novelli A Pampaloni 11092023 ROXIE Users Workshop 11092023 ROXIE Users Workshop ROXIE Version 1021 2D amp 3D magnet design . /SBS. – Front Tracker. PARAMETER. DESIGN VALUE. Microstrip. Silicon Detector. Number of tiles/plane and size. 2 @@@. Number of planes. 2. Size of. the single plane. @@@. Number of . microstrips. A.BalernaLaboratoriNazionalidiFrascati,INFN,viaE.Fermi40,00044Frascati,RM,Italye-mail:balerna@lnf.infn.itS.MobilioDipartimentodiScienze,Universita Kepler, . Ticho. Brahe, . Copernicus. Galileo, Newton. Einstein, . Eötvos. Amaldi. & the . resonating. . antennas. The era of . interferometers. : . . GEO600 & VIRGO in EU. . LIGO in USA, TAMA in Japan. European Gravitational Observatory. EGO. “Raison d'être”, origin, structure . & future perspectives. Federico Ferrini . – EGO Director. Welcome to. The Einstein Telescope. Design Study Presentation. Tracking particles in space and time. Very little help in the direction of this path is coming from nature, the burden is on the accelerator and experimental physicists to provide the means for this crossing.. DNS HA. A . multimaster. DNS configuration for Disaster Recovery and Business Continuity environment. HA DNS General Concepts. It is a fundamental component of a Disaster Recovery strategy . Objectives: . Polarization. B-. modes. . polarization. of the CMB: . produced. by . dark . matter. . structures. (. lensing. ) . crossed. by CMB . photons. Produced. by the . inflation. . process. in the . Gran . Sasso. Laboratori. . Nazionali. del Gran . Sasso. Stefano Ragazzi – INFN LNGS & UNIMIB. 3400 . m.w.e. .. 1.1 . μ / (m. 2 . h. ). Muon. flux: 3.0 10. -4. m. -2. s. -1. Neutron flux: . Pre. GDB . CERN, 10/1/2017. Stefano Zani. Stefano.Zani@cnaf.infn.it. 1. INFN CNAF data-center . CNAF runs the main . INFN computing . center providing . computing and storage services to ~30 scientific . New models for New models for PIXE simulation with Geant4 Maria Grazia Pia G. Weidenspointner,M. Augelli,L. Quintieri,P. Saracco, M. Sudhakar, A. Zoglauer INFNSidiGdINFNLbiNilidiFiIl INFN S G enova triennio. 2017-2019. N.Giglietto. Padova 18-19/11/2019. 1. Com’eravamo nel 2016. EoI. firmato nel 2015 (impegni base verso CTA). Premiale in conclusione (. sipm. ). Rapporti INAF-INFN in CTA. LST e SCT. Future silicon trackers:. 4D tracking. Nicolò. . Cartiglia. INFN - Italy. 2. N. Cartiglia, INFN. - KEK - Dec 12 2019 . Seminar will be set to 1 hour, so, 50 + 10 mins talk will be matched.. Most of audience will be experimental physicists.. – S. . Tomassini. – 06/24-25/2015. CLAS12 – RICH MECHANICS . REVIEW. SLIDE 1. RICH MODULE INTEGRATION IN CLAS_12 – LAST LAYOUT. RICH MODULE. INFN-LNF / D. . Orecchini. – S. . Tomassini. . Bozza. - University of Salerno / INFN – OBELICS F2F meeting Roma 26-27/1/2016. INFN in OBELICS. KM3NeT INFN groups. . Interested in tasks related to neutrino astronomy/astrophysics. . Interested in .

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